The Fermi Gamma-ray Observatory blind survey (FermiBlind) published its results in papers published from 2009 to 2018 with a total of 60 new pulsars discovered. It detected a grand total of 0 pulsars. The fastest pulsar discovered was J1311-3430 with a period of 2.56037 milliseconds and the slowest pulsar was J1057-5851 with a period of 620.36503 milliseconds.
The smallest pulsar dispersion measure was J1741-2054 with a DM of 4.7 pc/cc and the largest pulsar dispersion measure was J0002+6216 with a DM of 218.6 pc/cc. There were a total of 1838 pulsars known before the first discovery was published. This survey increased the total amount of known pulsars by 3.0%.
There were 8 papers written about the discoveries of this survey: Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT, Eight γ-ray Pulsars Discovered in Blind Frequency Searches of Fermi LAT Data, Precise γ-ray Timing and Radio Observations of 17 Fermi γ-ray Pulsars, PSR J0007+7303 in the CTA1 Supernova Remnant: New Gamma-Ray Results from Two Years of Fermi Large Area Telescope Observations, Discovery of Nine Gamma-Ray Pulsars in Fermi Large Area Telescope Data Using a New Blind Search Method, PSR J1838-0537: Discovery of a Young, Energetic Gamma-Ray Pulsar, Binary Millisecond Pulsar Discovery via Gamma-Ray Pulsations, Einstein@Home Discovery of Four Young Gamma-Ray Pulsars in Fermi LAT Data.